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Science 5 May 1989:
Vol. 244. no. 4904, pp. 564 - 566
DOI: 10.1126/science.11539817

Articles

Science, Vol 244, Issue 4904, 564-566
Copyright © 1989 by American Association for the Advancement of Science


articles

Diode-laser absorption spectroscopy of supersonic carbon cluster beams: the nu 3 spectrum of C5

Heath JR, AL Cooksy, MH Gruebele, CA Schmuttenmaer, and RJ Saykally

Department of Chemistry, University of California, Berkeley 94720, USA.

A new spectroscopic experiment has been developed in which rovibrational transitions of supersonically cooled carbon clusters, which were produced by laser vaporization of graphite, have been measured by direct-absorption diode-laser spectroscopy. Thirty-six sequential rovibrational lines of the nu 3 band of the C5 carbon cluster have been measured with Doppler-limited resolution. The absorption spectrum is characteristic of a linear molecule with a center of symmetry. Least-squares analysis of the spectrum indicates an effective carbon-carbon bond length of 1.283 angstroms, in good agreement with ab initio quantum chemical calculations. This work confirms the detection of C5 in IRC + 10216 reported in the accompanying paper.


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
Electron Photodetachment Cross Sections of Small Carbon Clusters: Evidence for Nonlinear Isomers.
D. Zajfman, H. Feldman, O. Heber, D. Kella, D. Majer, Z. Vager, and R. Naaman (1992)
Science 258, 1129-1131
   Abstract »    PDF »
The C7 cluster: structure and infrared frequencies.
J. Heath, R. Sheeks, A. Cooksy, and R. Saykally (1990)
Science 249, 895-897
   Abstract »    PDF »
Tunable far-IR laser spectroscopy of jet-cooled carbon clusters: the nu 2 bending vibration of C3.
C. Schmuttenmaer, R. Cohen, N Pugliano, Heath JR, A. Cooksy, K. Busarow, and R. Saykally (1990)
Science 249, 897-900
   Abstract »    PDF »
Detection of C5 in the Circumstellar Shell of IRC+10216.
P. F. BERNATH, K. H. HINKLE, and J. J. KEADY (1989)
Science 244, 562-564
   Abstract »    PDF »



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Science. ISSN 0036-8075 (print), 1095-9203 (online)